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rock > igneous rock > differentiated meteorite > differentiated achondrite > asteroidal achondrite > ureilite > mosaicized ureilite > Dyalpur
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Dyalpur
subjectfact 
Dyalpuris an instance of mosaicized ureilite2000-12-14 14:18:59.0
is an instance of meteorite fall2000-12-14 14:18:59.0
has olivine composition Fo% 842000-12-14 14:18:59.0
has pigeonite composition Wo% 11 En% 762000-12-14 14:18:59.0
has pyroxene content 0.41 in modal pyroxene/(pryroxene+olivine)2000-12-14 14:18:59.0
has reference Berkley et. al (1980)    has source: Berkley JL, Taylor GJ, Keil K. Harlow GE, Prinz M 1980, Geochim Cosmochim Acta 44, 1579, 2000-12-14 14:18:59.0
mosaicized ureilitehas texture mosaicized2000-12-14 14:18:45.0
has original texture visible via dark matrix outlining relict grain boundaries of large, elongate grains, and a common preferred orientation of grains within relict domains -has source: Berkley JL, Taylor GJ, Keil K. Harlow GE, Prinz M 1980, Geochim Cosmochim Acta 44, 1579 -has URL: http://adsabs.harvard.edu/cgi-bin/bib_query?1980GeCoA..44.1579B2000-12-14 14:18:45.0
has gain size much less than 1 mm2000-12-14 14:18:45.0
has shock pressure 100 GPa or greater2000-12-14 14:18:45.0
has shock diagnostic mineral diamonds and/or lonsdaleite2000-12-14 14:18:45.0
has olivine shock metamorphism completely shattered or mosaicized2000-12-14 14:18:45.0
has pyroxene shock metamorphism mottled by melt glass2000-12-14 14:18:45.0
meteorite fallhas fall date recorded by eyewitness or instruments2000-12-14 14:18:32.0
has value higher because the fall was witnessed2000-12-14 14:18:32.0
has fall description what witnesses saw or what was recorded by instruments2000-12-14 14:18:32.0
has weathering negligible due to quick recovery of meteorite before corrosion begins2000-12-14 14:18:32.0
ureilitehas letter designation AURE2000-12-14 14:18:43.0
has characteristic mineral olivine-pigeonite about 90% by volume2000-12-14 14:18:43.0
has matrix composition carbon, metal, sulfides small silicate grains along grain boundaries less than 10% by volume2000-12-14 14:18:43.0
has total mass of finds 9 kg (out of date)2000-12-14 14:18:43.0
has number of finds 6 (out of date)2000-12-14 14:18:43.0
has minerology olivine, pyroxene (some combination of pigeonite, orthopyroxene, augite)2000-12-14 14:18:43.0
has petrology coarse-grained granular2000-12-14 14:18:43.0
has likely origin partial melting residue2000-12-14 14:18:43.0
has olivine grain characteristic reduced rims contacting carbonaceous matrix material 0.1 mm FeO-free olivine and/or enstatite rims riddled with tiny inclusions of low-Ni metal2000-12-14 14:18:43.0
shock melted meteoritehas shock stage shock melted2000-12-14 14:18:46.0
has degree of shock metamorphism shock melted2000-12-14 14:18:46.0
meteoritehas fall location strewn fields, elongated footprints which depends on impact angle, airbursts, and impact velocity2000-12-14 14:18:31.0
has fall coordinates in degrees, minutes and seconds of lattitude and longitude2000-12-14 14:18:31.0
has fall map which appears as an elongated footprint which depends on impact angle, airbursts, and impact velocity2000-12-14 14:18:31.0
can have crater image2000-12-14 14:18:31.0
has original mass which can over an order of magnitude greater than total mass of fragment(s) collected at the impact site2000-12-14 14:18:31.0
has composition often minerals not found on Earth2000-12-14 14:18:31.0
has relative abundance2000-12-14 14:18:31.0
has total mass of finds 485755 kg2000-12-14 14:18:31.0
has number of finds 16912000-12-14 14:18:31.0
has impact velocity when it hits the ground which is smaller than its velocity before it enters the atmosphere2000-12-14 14:18:31.0
has impact angle2000-12-14 14:18:31.0
has weather resistance which depends on its composition2000-12-14 14:18:31.0
has monetary value large if the fall was witnessed2000-12-14 14:18:31.0
has name based on the locale, region, or nearby town in which the fall occurred2000-12-14 14:18:31.0
often produce power outages and failures in electrical equipment due to EMP (electromagnetic pulse)2000-12-14 14:18:31.0
can be associated with crater2000-12-14 14:18:31.0
has origin meteoroid from interplanetary space or fragment dislodged from another planet, moon or planetesimal2000-12-14 14:18:31.0
vaporizes completely if size is between 3 micrometers and 3 millimeters2000-12-14 14:18:31.0
can survive fall if size is larger than 3 mm and velocity is less than 24 km per second2000-12-14 14:18:31.0
can survive fall if it fragments because smaller pieces with less mass are more easily slowed by the atmosphere2000-12-14 14:18:31.0
has ablative mass loss depending on composition, more friable stony meteoroids loses more mass than iron meteoroid2000-12-14 14:18:31.0
has ablative mass loss directly proportional to initial velocity2000-12-14 14:18:31.0
can shatter during impact phase2000-12-14 14:18:31.0
can fragment during meteor phase2000-12-14 14:18:31.0
has fragmentation probability during meteor phase which depends on composition2000-12-14 14:18:32.0
shocked meteoritehas metamorphism mechanism shock metamorphism2000-12-14 14:18:46.0
rockhas part mineral2000-12-14 14:18:20.0
has genesis2000-12-14 14:18:20.0
plutonic rockhas solidification mechanism cooling in deep underground chambers2000-12-14 14:18:22.0
has solidification timescale very slow2000-12-14 14:18:22.0
achondritehas distinguishing feature no chondrules2000-12-14 14:18:42.0

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